The supernova-regulated ISM - VI. Magnetic effects on the structure of the interstellar medium

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dc.contributorAalto-yliopistofi
dc.contributorAalto Universityen
dc.contributor.authorEvirgen, C. C.
dc.contributor.authorGent, F. A.
dc.contributor.authorShukurov, A.
dc.contributor.authorFletcher, A.
dc.contributor.authorBushby, P. J.
dc.contributor.departmentNewcastle University
dc.contributor.departmentCentre of Excellence Research on Solar Long-Term Variability and Effects, ReSoLVE
dc.contributor.departmentDepartment of Computer Scienceen
dc.date.accessioned2019-09-25T14:13:27Z
dc.date.available2019-09-25T14:13:27Z
dc.date.issued2019-10
dc.description| openaire: EC/H2020/228398/EU//HPC-EUROPA2
dc.description.abstractWe explore the effect of magnetic fields on the vertical distribution and multiphase structure of the supernova-driven interstellar medium in simulations that admit dynamo action. As the magnetic field is amplified to become dynamically significant, gas becomes cooler and its distribution in the disc becomes more homogeneous. We attribute this to magnetic quenching of vertical velocity, which leads to a decrease in the cooling length of hot gas. A non-monotonic vertical distribution of the large-scale magnetic field strength, with the maximum at |z| approximate to 300pc causes a downward pressure gradient below the maximum which acts against outflow driven by SN explosions, while it provides pressure support above the maximum.en
dc.description.versionPeer revieweden
dc.format.extent10
dc.format.extent5065-5074
dc.format.mimetypeapplication/pdf
dc.identifier.citationEvirgen , C C , Gent , F A , Shukurov , A , Fletcher , A & Bushby , P J 2019 , ' The supernova-regulated ISM - VI. Magnetic effects on the structure of the interstellar medium ' Monthly Notices of the Royal Astronomical Society , vol. 488 , no. 4 , pp. 5065-5074 . https://doi.org/10.1093/mnras/stz2084en
dc.identifier.doi10.1093/mnras/stz2084
dc.identifier.issn0035-8711
dc.identifier.issn1365-2966
dc.identifier.otherPURE UUID: d2282115-2f95-4ede-a07b-b1a0b8a8bc06
dc.identifier.otherPURE ITEMURL: https://research.aalto.fi/en/publications/the-supernovaregulated-ism--vi-magnetic-effects-on-the-structure-of-the-interstellar-medium(d2282115-2f95-4ede-a07b-b1a0b8a8bc06).html
dc.identifier.otherPURE FILEURL: https://research.aalto.fi/files/37080644/stz2084.pdf
dc.identifier.urihttps://aaltodoc.aalto.fi/handle/123456789/40472
dc.identifier.urnURN:NBN:fi:aalto-201909255493
dc.language.isoenen
dc.publisherOXFORD UNIV PRESS INC
dc.relationinfo:eu-repo/grantAgreement/EC/H2020/228398/EU//HPC-EUROPA2
dc.relation.ispartofseriesMonthly Notices of the Royal Astronomical Societyen
dc.relation.ispartofseriesVolume 488, issue 4en
dc.rightsopenAccessen
dc.subject.keywordMHD
dc.subject.keywordturbulence
dc.subject.keywordISM: evolution
dc.subject.keywordgalaxies: kinematics and dynamics
dc.subject.keywordgalaxies: magnetic fields
dc.subject.keywordCOSMIC-RAY
dc.subject.keywordHYDROSTATIC EQUILIBRIUM
dc.subject.keywordTURBULENT MODEL
dc.subject.keyword3-DIMENSIONAL EVOLUTION
dc.subject.keywordDYNAMICAL EVOLUTION
dc.subject.keywordDIRECT SIMULATIONS
dc.subject.keywordGALACTIC WINDS
dc.subject.keywordSTAR-FORMATION
dc.subject.keywordGLOBAL-MODELS
dc.subject.keywordDRIVEN
dc.subject.keyword113 Computer and information sciences
dc.subject.other113 Computer and information sciencesen
dc.titleThe supernova-regulated ISM - VI. Magnetic effects on the structure of the interstellar mediumen
dc.typeA1 Alkuperäisartikkeli tieteellisessä aikakauslehdessäfi
dc.type.versionpublishedVersion

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